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arXiv · 1504.01348

DBI Galileon inflation in the light of Planck 2015

K. Sravan Kumar·Juan C. Bueno Sanchez·Celia Escamilla-Rivera·Joao Marto·Paulo Vargas Moniz
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Abstract

In this work we consider a DBI Galileon (DBIG) inflationary model and constrain its parameter space with the Planck 2015 and BICEP2/Keck array and Planck (BKP) joint analysis data by means of a potential independent analysis. We focus our attention on inflationary solutions characterized by a constant or varying sound speed as well as warp factor. We impose bounds on stringy aspects of the model, such as the warp factor $\left(f\right)$ and the induced gravity parameter $\left(\tilde{m}\right)$. We study the parameter space of the model and find that the tensor-to-scalar ratio can be as low as $r\simeq6\times10^{-4}$ and inflation happens to be at GUT scale. In addition, we obtain the tilt of the tensor power spectrum and test the standard inflationary consistency relation $\left(r=-8n_{t}\right)$ against the latest bounds from the combined results of BKP+Laser Interferometer Gravitational-Waves Observatory (LIGO), and find that DBIG inflation predicts a red spectral index for the tensor power spectrum.

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K. Sravan Kumar, Juan C. Bueno Sanchez, Celia Escamilla-Rivera, Joao Marto, Paulo Vargas Moniz. 2016-02-27. DBI Galileon inflation in the light of Planck 2015. https://doi.org/10.1088/1475-7516%2F2016%2F02%2F063

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